[21.14] The Nuclear Stellar Dynamics of the S0 Galaxy NGC7332

STIS near-IR longslit spectroscopy of the nearby S0 galaxy
NGC 7332 was obtained of the Ca II triplet absorption lines
at ~8600 Å. We use the Fourier correlation quotient
method (Bender 1990, A&Ap, 229, 441) to extract the
line-of-sight velocity distribution in the inner 4\prime
\prime of the galaxy. Combined with ground-based imaging
and spectroscopy (Fisher, Illingworth & Franx 1994, AJ,
107, 160) and HST WF/PC-1 imaging (Lauer et al. 1995,
AJ, 110, 2622) these data were fitted with three-integral
dynamical models developed by K. Gebhardt, to investigate
the nuclear stellar dynamics and to search for evidence of a
massive black hole. Since Maggorian et al. (1998, AJ,
115, 2285) find it to be the best case for M\bullet=0,
NGC 7332 is an important object.